Part 3

Differential Geometry

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Problem 3.1.1

Let α(s)\alpha (s) be a closed plane curve. Define the diameter dαd_\alpha of α(s)\alpha (s) to be

dα=sup⁡t,s∈R∥α(s)−α(t)∥. d_\alpha = \sup _{t,s \in \mathbb {R}} \left\| \alpha (s) - \alpha (t)\right\| .

Now assume that the curvature k(s)≥1k(s) \geq 1 for all ss.

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(a)

For any N∈Z+N \in \mathbb {Z}^+ sketch an example of such an α(s)\alpha (s) with dα>Nd_\alpha > N.

(b)

Assume further that α\alpha is a simple closed curve. Prove that dα≤2d_\alpha \leq 2 (or some other constant independent of α\alpha; 2 is the best possible such constant).

Problem 3.1.2

Let α\alpha be a regular C∞C^\infty curve in R3\mathbb {R}^{3} with nonvanishing curvature. Suppose the normal vector N(t)N(t) is proportional to the position vector; that is, N(t)=c(t)α(t)N(t) = c(t)\alpha (t) for all tt, where cc is a smooth function. Determine all such curves.

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Problem 3.1.3

A surface S⊂R3S \subset \mathbb {R}^{3} is called triply ruled if at every p∈Sp \in S we can find three open line segments L1,L2,L3L_1, L_2, L_3 lying in SS such that L1∩L2∩L3={p}L_1 \cap L_2 \cap L_3 = \{ p\}. Determine all triply ruled surfaces.

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Problem 3.1.4

Let γ:(a,b)→R3\gamma : (a,b) \to \mathbb {R}^{3} be smooth with ∣γ′∣=1\left|\gamma '\right| = 1 and curvature kk and torsion τ\tau, both nonvanishing. Denote the Frenet frame by {T,N,B}\{ T, N, B\}. Assume that there exists a unit vector a∈R3a \in \mathbb {R}^{3} with

T⋅a=constant=cos⁡α. T \cdot a = \text{constant} = \cos \alpha .
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(a)

Show that a circular helix is an example of such a curve.

(b)

Show that N⋅a=0N \cdot a = 0.

(c)

Show that k/τ=constant=±tan⁡αk/\tau = \text{constant} = \pm \tan \alpha.

Problem 3.1.5

Show that if γ\gamma is a geodesic on the cone z=x2+y2z = \sqrt{x^2+y^2}, (x,y)∈R2∖{(0,0)}(x,y) \in \mathbb {R}^{2} \setminus \{ (0,0)\}, then γ\gamma intersects itself at most a finite number of times.

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Problem 3.1.6

Let γ:(a,b)→R3\gamma : (a,b) \to \mathbb {R}^{3} be a C∞C^\infty curve parameterized by arc length, with curvature and torsion k(s)k(s) and τ(s)\tau (s). Assume k(s)≠0k(s) \neq 0, τ(s)≠0\tau (s) \neq 0 for all s∈(a,b)s \in (a,b), and let TT and NN denote the unit tangent and normal vectors to γ\gamma. The curve γ\gamma is called a Bertrand curve if there exists a regular curve γˉ:(a,b)→R3\bar\gamma : (a,b) \to \mathbb {R}^{3} such that for each s∈(a,b)s \in (a,b) the normal lines of γ\gamma and γˉ\bar\gamma at ss are equal. In this case, γˉ\bar\gamma is called the Bertrand mate of γ\gamma and we can write γˉ(s)=γ(s)+rN(s)\bar\gamma (s) = \gamma (s) + rN(s) for some r=r(s)∈Rr = r(s) \in \mathbb {R}. (Note that ss might not be an arc length parameter for γˉ\bar\gamma.)

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(a)

Prove that rr is constant.

(b)

Prove that if γ\gamma is a Bertrand curve (with rr as above), then there exists a constant CC such that rk(s)+Cr(s)=1rk(s) + Cr(s) = 1 for all s∈(a,b)s \in (a,b).

(c)

Prove that if γ\gamma has more than one Bertrand mate, then γ\gamma is a circular helix.

Problem 3.1.7

Let x(s)x(s) be a curve in R3\mathbb {R}^{3} parameterized by arc-length. Assume that τ(s)≠0\tau (s) \neq 0 and k′(s)≠0k'(s) \neq 0 for all ss. Show that a necessary and sufficient condition for x(s)x(s) to lie on a sphere is that

1k2(s)+1τ2(s)⋅k′2(s)k4(s)=constant. \frac{1}{k^2(s)} + \frac{1}{\tau ^2(s)} \cdot \frac{k'^2(s)}{k^4(s)} = \text{constant}.
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Problem 3.1.8

Let M⊂R3M \subset \mathbb {R}^{3} be the torus obtained by rotating the circle {(0,y,z):(y−2)2+z2=1}\{ (0, y, z) : (y-2)^2 + z^2 = 1\} around the zz-axis, and let c(t)=(2cos⁡t,2sin⁡t,1)c(t) = (2\cos t, 2 \sin t, 1) ("top circle"). Is this curve a geodesic on MM? Explain without long computations.

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Problem 3.1.9

Let γ:[0,1]→R3\gamma : [0,1] \to \mathbb {R}^{3} be a C∞C^\infty curve with ∣γ′∣=1\left|\gamma '\right| = 1 and non-vanishing curvature. Assume the torsion τ≡0\tau \equiv 0.

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(a)

Show that γ\gamma lies in a plane.

(b)

What happens if the curvature is allowed to vanish at a point?

Problem 3.1.10

Let f:R→Rf : \mathbb {R} \to \mathbb {R} be positive and smooth. Let MM be the surface in R3\mathbb {R}^{3} obtained by rotating the graph {(x,f(x)):x∈R}\{ (x, f(x)) : x \in \mathbb {R}\} of ff in the xzxz plane about the xx axis. Characterize in terms of ff the set of xx such that 1f(x)\dfrac {1}{f(x)} is a principal curvature of MM at (x,0,f(x))(x, 0, f(x)).

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Problem 3.1.11

Let α(s)⊂R3\alpha (s) \subset \mathbb {R}^{3} be a smooth curve parameterized by arc-length. Assume that the position vector α(s)\alpha (s) is always a linear combination of the binormal and normal vectors B(s),N(s)B(s), N(s) of α(s)\alpha (s). Show that α(s)\alpha (s) does not pass through O∈R3O \in \mathbb {R}^{3}.

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Problem 3.1.12

Let M2⊂R3M^2 \subset \mathbb {R}^{3} be the cylinder x2+y2=1x^2+y^2=1. Suppose the curve α(s)⊂M2\alpha (s) \subset M^2 is parameterized by arclength.

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(a)

If k(s)>0k(s) > 0 and τ(s)=0\tau (s) = 0, show that α(s)\alpha (s) is a closed curve. (Here k,τk, \tau are curvature and torsion of α\alpha in R3\mathbb {R}^{3}.)

(b)

If kg(s)=1k_g(s) = 1, show that α(s)\alpha (s) is a closed curve (kgk_g is the geodesic curvature in MM).

Problem 3.1.13

Let Γ\Gamma be a two-dimensional distribution in R3\mathbb {R}^{3} defined by

Γ(x,y,z)=⟨∂∂x−y∂∂z, ∂∂y⟩. \Gamma _{(x,y,z)} = \left\langle \frac{\partial }{\partial x} - y \frac{\partial }{\partial z}, \, \frac{\partial }{\partial y}\right\rangle .
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(a)

Show that Γ\Gamma is not involutive.

(b)

Given a C∞C^\infty curve α(s)⊂R2={(x,y,0):x,y∈R}⊂R3\alpha (s) \subset \mathbb {R}^{2} = \{ (x,y,0) : x, y \in \mathbb {R}\} \subset \mathbb {R}^{3} and β(s0)\beta (s_0), show that there exists a unique C∞C^\infty curve β(s)⊂R3\beta (s) \subset \mathbb {R}^{3} such that β′(s)∈Γβ(s)\beta '(s) \in \Gamma_{\beta (s)}, β(s0)=α(s0)\beta (s_0) = \alpha (s_0) and π(β(s))=α(s)\pi (\beta (s)) = \alpha (s), where π(x,y,z)=(x,y,0)\pi (x,y,z) = (x,y,0).

(c)

Show that if α(s)\alpha (s) is a simple closed curve of length LL bounding the region Ω\Omega in R2\mathbb {R}^{2}, then β(s0+L)−β(s0)=(0,0,±A)\beta (s_0 + L) - \beta (s_0) = (0, 0, \pm A) where A=A = area of Ω\Omega.

Problem 3.1.14

Call a normal vector field vv along a space curve γ\gamma parallel if v′v' is always tangent to γ\gamma.

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(a)

Show that the angle through which a parallel normal vector field vv turns relative to the principal normal NN along γ\gamma is given by the total torsion of γ\gamma, i.e.,

θ(L)−θ(0)=∫0Lτ(s) ds. \theta (L) - \theta (0) = \int _0^L \tau (s) \, ds.

Here ss and LL denote arclength and the length of γ\gamma, respectively.

(b)

Show that the total torsion of any closed curve γ\gamma which lies on a sphere in R3\mathbb {R}^{3} must vanish.

Problem 3.1.15

Let MM be a surface in R3\mathbb {R}^{3} and let PP be a plane. Suppose MM and PP intersect orthogonally. Show that the intersection curve (parameterized by arclength) is a geodesic on MM.

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Problem 3.1.16

Let α(s)\alpha (s) be a C2C^2 curve in R3\mathbb {R}^{3} parameterized by arclength. Suppose that for some function f(s)f(s), α′′(s)=f(s)α(s)\alpha ''(s) = f(s)\alpha (s). What can you deduce about f(s)f(s), α(s)\alpha (s)?

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Problem 3.1.17

Suppose γ(t)\gamma (t) parameterizes a space curve with curvature function ρ(t)\rho (t). Define a new curve γˉ\bar\gamma by setting, for each t∈Rt \in \mathbb {R}, γˉ(t):=cγ(t/c)\bar\gamma (t) := c\gamma (t/c), where c∈Rc \in \mathbb {R} is an arbitrary fixed constant. Derive the curvature function for this new curve.

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Problem 3.1.18

Let α:(a,b)→R3\alpha : (a,b) \to \mathbb {R}^{3} be a smooth curve with non-vanishing curvature.

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(a)

Show that if the torsion of α\alpha vanishes identically then there is a plane π⊂R3\pi \subset \mathbb {R}^{3} containing α\alpha, that is, α(t)∈π\alpha (t) \in \pi for all t∈(a,b)t \in (a,b). Is π\pi unique?

(b)

Is the conclusion of (a) still true if the curvature is allowed to vanish at a single point c∈(a,b)c \in (a,b)?

[Of course, the torsion is not defined at cc, but is assumed to be zero at all other points.]

Problem 3.1.19

Let α\alpha and β\beta be two regular curves in R3\mathbb {R}^{3}. The curve β\beta is called an involute of α\alpha if for all tt, β(t)\beta (t) lies on the line tangent to α\alpha at α(t)\alpha (t) and ⟨α′(t),β′(t)⟩=0\left\langle \alpha '(t), \beta '(t) \right\rangle = 0. Show that every involute of a generalized helix α\alpha is a plane curve. (Recall that α\alpha is a generalized helix if for some constant vector u≠0u \neq 0, ⟨u,α′(s)⟩=const\left\langle u, \alpha '(s) \right\rangle = \text{const}, where ss is arclength for α\alpha.)

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Problem 3.1.20

Suppose that the unit normal vector to a surface M⊂R3M \subset \mathbb {R}^{3} is constant along a regular curve α⊂M\alpha \subset M. Deduce that in this case, α\alpha is an asymptotic curve, that a plane contains it, and that the Gauss curvature of MM vanishes at each point of α\alpha.

[Note: A curve in a surface is called asymptotic if its acceleration is everywhere tangent to that surface.]

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Problem 3.1.21

Sketch the closed regular plane curve β:[−π,π]→R2\beta : [-\pi , \pi ] \to \mathbb {R}^{2} having β(0)=(0,0)\beta (0) = (0,0) and β′(0)=(1,0)\beta '(0) = (1,0), if β\beta's curvature function k(s)k(s) (s=s = arclength) is odd, satisfies

∫0πk(s) ds=3π/2, \int _0^\pi k(s) \, ds = 3\pi /2,

and has the following graph. (Include an explanation with your sketch.)

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Problem 3.1.22

Let X⊂R2X \subset \mathbb {R}^{2} be a connected one-dimensional real analytic submanifold, not contained in a line. Prove that not every tangent line to XX is bitangent -- that is, it is not the case that for all p∈Xp \in X there exists q≠pq \neq p such that the tangent line to XX at pp equals the tangent line to XX at qq as lines in R2\mathbb {R}^{2}.

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Problem 3.2.1
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(a)

Show that there exists a metric on the plane so that some geodesics are simple closed curves.

(b)

Let α(s)\alpha (s) be a simple closed geodesic as described above and K(x)K(x) be the Gaussian curvature of the above metric at x∈R2x \in \mathbb {R}^{2}. Compute

∫interior of αK. \int _{\text{interior of } \alpha } K.

Here the integral is with respect to the Riemannian volume induced by the metric.

Problem 3.2.2

Let M2⊂R3M^2 \subset \mathbb {R}^{3} be a surface containing x=0x=0. Assume that ∂∂x1\dfrac {\partial }{\partial x_1} and ∂∂x2\dfrac {\partial }{\partial x_2} are tangent to MM at x=0x=0, and that in that basis the Weingarten map

L=(433−4). L = \begin{pmatrix} 4 & 3 \\ 3 & -4 \end{pmatrix}.

Let α\alpha be the curve (near x=0x=0) obtained by intersecting MM with the x1x3x_1x_3 plane.

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(a)

What is the normal curvature of α\alpha at x=0x=0?

(b)

What is the geodesic curvature of α\alpha at x=0x=0?

(c)

What is the Gaussian curvature of M2M^2 at x=0x=0?

(d)

Sketch the surface near x=0x=0. You may assume that the normal to the surface at x=0x=0 is (0,0,1)(0,0,1).

Problem 3.2.3

Let M={(x,y,z)∈R3:z=6−(x2+y2)}M = \{ (x,y,z) \in \mathbb {R}^{3} : z = 6 - (x^2+y^2)\} (a paraboloid of revolution). D={(x,y,z)∈M:z>2}D = \{ (x,y,z) \in M : z > 2\}, and ω=yz2 dx+xz dy+x2y2 dz\omega = yz^2 \, dx + xz \, dy + x^2y^2 \, dz. Orient MM and evaluate

∫Dz dx∧dy+dω. \int _D z \, dx \wedge dy + d\omega .
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Problem 3.2.4

Let SS be a surface diffeomorphic to the ordinary 2-sphere. Suppose there is a C∞C^\infty metric of positive curvature on SS for which there exist two simple closed geodesics γ1\gamma_1 and γ2\gamma_2. Show that γ1\gamma_1 and γ2\gamma_2 must intersect.

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Problem 3.2.5

Let DD be the disk {(x,y)∈R2:x2+y2<14}\{ (x,y) \in \mathbb {R}^{2} : x^2+y^2 < \tfrac 14\} and let O=(0,0)∈DO = (0,0) \in D. Let (x1,x2)=(r,θ)(x_1,x_2) = (r,\theta ) be the usual polar coordinates and define a metric on D∖{O}D\setminus \{ O\} by

(gij)=(100h(r,θ)), (g_{ij}) = \begin{pmatrix} 1 & 0 \\ 0 & h(r,\theta ) \end{pmatrix},

where h(r,θ)=r2[1−2r2+r4sin⁡2θ]2h(r,\theta ) = r^2[1 - 2r^2 + r^4\sin^2\theta ]^2.

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(a)

Prove that this metric extends to a smooth metric on DD.

(b)

Show that line segments in DD which pass through the origin (suitably parameterized) are geodesics.

Problem 3.2.6
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(a)

Let MM be a surface (without boundary) in R3\mathbb {R}^{3}. Suppose MM is inside a ball of radius RR and suppose a point p∈Mp \in M is on the boundary sphere. Show that the Gauss curvature of MM at pp is ≥1R2\geq \dfrac {1}{R^2}.

(b)

Show that there is no closed minimal surface in R3\mathbb {R}^{3}.

Problem 3.2.7

Let H2={(x,y)∈R2,y>0}H^2 = \{ (x,y) \in \mathbb {R}^{2}, y > 0\} be the upper half-plane in R2\mathbb {R}^{2} and let H2H^2 have the Riemannian metric gg such that

g(x,y)=1y2(x,y)for (x,y)∈H2, g(x,y) = \frac{1}{y^2}(x,y) \quad \text{for } (x,y) \in H^2,

where (x,y)(x,y) is the usual inner product on R2\mathbb {R}^{2}.

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(a)

Compute the components of the Levi--Civita connection (i.e., the Christoffel symbols).

(b)

Let V(0)=(0,1)V(0) = (0,1) be a tangent vector at the point (0,1)∈H2(0,1) \in H^2. Let V(t)=(a(t),b(t))V(t) = (a(t), b(t)) be the parallel transport of V(0)V(0) along the curve x=tx=t, y=1y=1. Show that V(t)V(t) makes an angle tt with the direction of the yy-axis in the clockwise direction.

Problem 3.2.8

Consider the hyperboloid SS of one sheet x2+y2−z2=4x^2+y^2-z^2=4.

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(a)

Define the Gauss curvature KK of SS.

(b)

Use the definition from part (a) to compute KK at (0,2,0)(0,2,0).

Problem 3.2.9

Calculate the total geodesic curvature of a circle of radius rr on a sphere of radius R>rR > r.

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Problem 3.2.10

Let SS be an embedded closed surface in R3\mathbb {R}^{3} with the position vector X(p)X(p) and the unit outward normal vector N(p)N(p) for p∈Sp \in S. For a fixed (small) tt, define a surface StS_t to be the set St={X(p)+tN(p)∈R3∣p∈S}S_t = \{ X(p) + tN(p) \in \mathbb {R}^{3} \mid p \in S\}. Let κ1,κ2\kappa_1, \kappa_2 be the principal curvatures of SS at the point pp with respect to the outward normal vector. Let HtH_t be the mean curvature of StS_t at the point X(p)+tN(p)X(p)+tN(p) with respect to the outward normal vector (mean curvature is defined to be the sum of the two principal curvatures). Show that

Ht=κ11−tκ1+κ21−tκ2. H_t = \frac{\kappa _1}{1-t\kappa _1} + \frac{\kappa _2}{1-t\kappa _2}.
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Problem 3.2.11

Let λ:R→R\lambda : \mathbb {R} \to \mathbb {R} be a smooth function with compact support, and consider the Riemannian surface obtained by equipping R2\mathbb {R}^{2} with a metric gg of the form

g(v→,w→):=eλ(y)⟨v→,w→⟩ g(\overrightarrow {v}, \overrightarrow {w}) := e^{\lambda (y)} \left\langle \overrightarrow {v}, \overrightarrow {w} \right\rangle

for v→,w→∈T(x,y)R2\overrightarrow {v}, \overrightarrow {w} \in T_{(x,y)}\mathbb {R}^{2}. Assuming the Gauss curvature KK of this metric is everywhere non-negative, use the Gauss--Bonnet Theorem to deduce that in fact, the surface is flat.

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Problem 3.2.12

Let M2⊂R3M^2 \subset \mathbb {R}^{3} be a smooth compact surface such that M2⊂{(x,y,z):z≥0}M^2 \subset \{ (x,y,z) : z \geq 0\}. Assume that M2∩{(x,y,z):z=0}M^2 \cap \{ (x,y,z) : z=0\} is a smooth curve α(s)\alpha (s), parameterized by arclength.

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(a)

Show that α(s)\alpha (s) is an asymptotic curve on M2M^2.

(b)

Show that α′(s)\alpha '(s) is always a principal direction.

(c)

Let us now drop the assumption that M2∩{(x,y,z):z=0}M^2 \cap \{ (x,y,z) : z=0\} is a curve. What kind of a set could M2∩{(x,y,z):z=0}M^2 \cap \{ (x,y,z) : z=0\} be?

Problem 3.2.13
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(a)

Construct an example of a non-compact C∞C^\infty surface in R3\mathbb {R}^{3} with a sequence of closed geodesics {σi}\{ \sigma_i\} such that length(σi)→0(\sigma_i) \to 0.

(b)

Show that this is not possible if the surface is compact.

Problem 3.2.14

Let (r(s),0,z(s))(r(s), 0, z(s)) be a unit speed curve in R3\mathbb {R}^{3} with r(s)>0r(s) > 0. Consider the surface of revolution (s,θ)→(r(s)cos⁡θ,r(s)sin⁡θ,z(s))(s,\theta ) \to (r(s)\cos \theta , r(s)\sin \theta , z(s)). On this surface compute the covariant derivatives ∇∂∂θ∂∂s\nabla_{\frac{\partial }{\partial \theta }}\frac{\partial }{\partial s} and ∇∂∂θ∂∂θ\nabla_{\frac{\partial }{\partial \theta }}\frac{\partial }{\partial \theta } in terms of ∂∂θ\frac{\partial }{\partial \theta } and ∂∂s\frac{\partial }{\partial s}.

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Problem 3.2.15

Let M2⊂R3M^2 \subset \mathbb {R}^{3} be an embedded compact surface of genus ≥1\geq 1. Show that the Gauss curvature of MM must vanish somewhere on MM.

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Problem 3.2.16

Consider the torus-of-revolution TT obtained by rotating the circle (x−a)2+z2=r2(x-a)^2+z^2=r^2 around the zz-axis:

T={(x,y,z):(x2+y2+z2+a2−r2)2−4a2(x2+y2)=0}. T = \{ (x,y,z) : (x^2+y^2+z^2+a^2-r^2)^2 - 4a^2(x^2+y^2) = 0\} .

Parameterize this torus, compute its Gauss curvature function KK, and verify that ∫TK dA=0\int_T K \, dA = 0 by explicit calculation.

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Problem 3.2.17

Let

x(t)=(12cos⁡t,12sin⁡t,32),0≤t<2π x(t) = \left(\frac12\cos t, \frac12\sin t, \frac{\sqrt3}{2}\right), \qquad 0 \leq t < 2\pi

be a curve on S2⊂R3S^2 \subset \mathbb {R}^{3}. Let X0=∂∂x2∈T(12,0,32)S2X_0 = \dfrac {\partial }{\partial x_2} \in T_{\left(\frac12,0,\frac{\sqrt3}{2}\right)} S^2. Compute the parallel translation of X0X_0 along x(t)x(t).

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Problem 3.2.18

Show that for any Riemannian metric on S2S^2 with ∣K∣≤1\left|K\right| \leq 1, where KK is the Gauss curvature, the area of S2S^2 is not less than 4π4\pi.

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Problem 3.2.19

Define "geodesics", and characterize (with proof):

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(a)

All geodesics on the unit sphere S2⊂R3S^2 \subset \mathbb {R}^{3}.

(b)

All geodesics on the surface {(x,y,z)∈R3:x2+y2≡1}\{ (x,y,z) \in \mathbb {R}^{3} : x^2+y^2 \equiv 1\}.

Problem 3.2.20

Give an example (e.g., draw a picture) to show that a connected surface can have two points which are not joined by any geodesic. What is the usual topological hypothesis that prevents this problem?

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Problem 3.2.21

Define "minimal surface in R3\mathbb {R}^{3}", and prove that the catenoid, obtained by rotating the graph of y=cosh⁡(x)y = \cosh (x) around the xx-axis in R3\mathbb {R}^{3}, is minimal.

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Problem 3.2.22

The "Clifford" torus in S3S^3 can be parameterized using charts of the form

X(u,v)=12(cos⁡u,sin⁡u,cos⁡v,sin⁡v) X(u,v) = \frac{1}{\sqrt2}(\cos u, \sin u, \cos v, \sin v)

where uu and vv are constrained to lie within intervals length <2π< 2\pi.

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(a)

Compute the metric [gij][g_{ij}] on the Clifford torus for a coordinate chart of the indicated type.

(b)

Figure out the Clifford torus' Gauss curvature function.

(c)

Deduce from the result of (b) that the Euler characteristic of a torus is zero.

Problem 3.2.23

Let f:R2→Rf : \mathbb {R}^{2} \to \mathbb {R} be a smooth function with a critical point (e.g., a minimum or maximum) at the origin x1=x2=0x_1=x_2=0.

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(a)

Show that the principal curvatures of the graph

z=f(x1,x2) z = f(x_1,x_2)

at (0,0,f(0,0))∈R3(0,0,f(0,0)) \in \mathbb {R}^{3} are the same as the eigenvalues of the Hessian matrix [∂2f/∂xi∂xj][\partial^2 f/\partial x_i \partial x_j] at (0,0)(0,0).

(b)

Show that R3\mathbb {R}^{3} contains no compact embedded surface with strictly negative Gauss curvature at all its points.

Problem 3.2.24

Let MM be a 2-dimensional manifold smoothly embedded in R3\mathbb {R}^{3} with unit normal nn.

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(a)

Prove that for each p∈Mp \in M there exist an open neighborhood UpU_p of pp in R3\mathbb {R}^{3} and a smooth function F:Up→RF : U_p \to \mathbb {R} such that F−1(0)=Up∩MF^{-1}(0) = U_p \cap M.

(b)

Find FF if MM is the graph of a smooth function f:R2→Rf : \mathbb {R}^{2} \to \mathbb {R}.

Problem 3.2.25

Let MM be a 2-dimensional manifold smoothly embedded in R3\mathbb {R}^{3} with unit normal nn. Assume that MM is the boundary of a bounded convex open set. Assume that nn is the exterior normal and that the Gauss curvature KK of MM is everywhere positive. [Recall that S⊆R3S \subseteq \mathbb {R}^{3} is defined to be convex if for each two points of SS the line segment joining these points lies in SS. You may use without proof the fact that MM lies on one side of each of its tangent planes.]

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(a)

Define the Gauss (or sphere) map

η:M→S2={(x,y,z):x2+y2+z2=1}. \eta : M \to S^2 = \{ (x,y,z) : x^2+y^2+z^2=1\} .
(b)

Prove that η\eta is one-to-one.

(c)

Assuming that η\eta is one-to-one, prove that η\eta is a diffeomorphism onto S2S^2.

(d)

Show that

∫MK(p) dp=4π. \int _M K(p) \, dp = 4\pi .

(You may assume (b) and (c) if you wish.)

Problem 3.2.26

Let MM be a 2-dimensional manifold smoothly embedded in R3\mathbb {R}^{3} with unit normal nn.

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(a)

Explain what is meant by intrinsic and extrinsic quantities on MM.

(b)

Are the principal curvatures intrinsic?

(c)

Discuss why the covariant derivative on MM, defined using the covariant derivative on R3\mathbb {R}^{3}, is intrinsic.

(d)

Assuming (c), discuss why the Gauss curvature of MM is intrinsic.

Problem 3.2.27

By revolving the curve γ\gamma sketched below around the xx-axis, we get a surface of revolution M2⊂R3M^2 \subset \mathbb {R}^{3}. Compute ∫MK dA\int_M K \, dA, where KK is the Gauss curvature and dAdA the area form, on MM. (Make sure to justify your answer.)

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Problem 3.2.28

A surface Σ2\Sigma^2 immersed in a Riemannian manifold NN is said to be ruled if it can be parameterized near any point by a mapping X:(0,1)2→NX : (0,1)^2 \to N such that for each fixed v0∈(0,1)v_0 \in (0,1), the uu-parameter curve X(u,v0)X(u,v_0) is a geodesic in NN.

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(a)

When n=3n=3, show that the Gauss curvature of a ruled surface in Rn\mathbb {R}^{n} is nowhere positive.

(b)

Show it for arbitrary nn.

Problem 3.2.29

Let α:(0,1)→R3\alpha : (0,1) \to \mathbb {R}^{3} be any regular arc (that is, α\alpha is differentiable and α′\alpha ' is nowhere zero). Let T(u),N(u)T(u), N(u) and B(u)B(u) be the unit tangent, normal and binormal vectors to α\alpha at α(u)\alpha (u). Consider the normal tube of radius ε\varepsilon around α\alpha, that is, the surface given parametrically by ϕ(u,v)=α(u)+εcos⁡(v)N(u)+εsin⁡(v)B(u)\phi (u,v) = \alpha (u) + \varepsilon \cos (v) N(u) + \varepsilon \sin (v) B(u).

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(a)

For what values of ε\varepsilon is this an immersion?

(b)

Assuming that α\alpha itself has finite length, find the surface area of the normal tube of radius ε\varepsilon around α\alpha.

Problem 3.2.30

Show that the ellipsoid x2+2y2+3z2=1x^2+2y^2+3z^2=1 is not isometric to any sphere x2+y2+z2=r2x^2+y^2+z^2=r^2.

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Problem 3.2.31

Let (f(v)cos⁡(u),f(v)sin⁡(u),g(v))(f(v)\cos (u), f(v)\sin (u), g(v)) be a parametrization of a surface of revolution S⊂R3S \subset \mathbb {R}^{3} where (u,v)∈(0,2π)×(a,b)(u,v) \in (0,2\pi )\times (a,b). If SS is given the induced metric from R3\mathbb {R}^{3}, prove that the following map from SS to R2\mathbb {R}^{2} is locally conformal where R2\mathbb {R}^{2} is given the standard Euclidean metric:

(u,v)↦(u,∫(f′(v))2+(g′(v))2f(v) dv). (u,v) \mapsto \left(u, \int \frac{\sqrt{(f'(v))^2+(g'(v))^2}}{f(v)} \, dv\right).
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Problem 3.2.32

Let SS be a smooth surface in R3\mathbb {R}^{3} defined by r(u,v)r(u,v), where rr is the radius vector of R3\mathbb {R}^{3} and (u,v)(u,v) are curvilinear coordinates on SS. Let HH and KK be respectively the mean curvature and the Gaussian curvature of SS. Let AA and BB be respectively the supremum of the absolute value of HH and KK on SS. Let aa be a positive number and nn be the unit normal vector of SS. Consider the surface S~\tilde S defined by ρ(u,v)=r(u,v)+an(u,v)\rho (u,v) = r(u,v) + a n(u,v). Let CC be a curve in SS defined by u=u(t)u=u(t) and v=v(t)v=v(t). Let C~\tilde C be the curve in S~\tilde S defined by t→ρ(u(t),v(t))t \to \rho (u(t),v(t)). Show that the length of C~\tilde C is no less than the length of CC multiplied by 1−a(A+A2+4B)1-a(A+\sqrt{A^2+4B}).

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Problem 3.2.33

Let u↦ρ(u)u \mapsto \rho (u) be a smooth curve in R3\mathbb {R}^{3}. Let SS be the surface in R3\mathbb {R}^{3} defined by (u,v)↦ρ(u)+vρ′(u)(u,v) \mapsto \rho (u) + v\rho '(u), where ρ′(u)\rho '(u) means the first-order derivative of ρ(u)\rho (u) with respect to uu. Assume that the two vectors ρ′(u)\rho '(u) and ρ′(u)+vρ′′(u)\rho '(u) + v\rho ''(u) are R\mathbb {R}-linearly independent at the point (u,v)=(u0,v0)(u,v) = (u_0,v_0), where ρ′′(u)\rho ''(u) means the second-order derivative of ρ(u)\rho (u) with respect to uu. Verify directly from the definition of Gaussian curvature that the Gaussian curvature of SS is zero at the point (u,v)=(u0,v0)(u,v) = (u_0,v_0).

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Problem 3.2.34

Let M2⊂R3M^2 \subset \mathbb {R}^{3} be an embedded oriented surface and let S2S^2 be the unit sphere. The Gauss map G:M→S2G : M \to S^2 is defined to be G(x)=N(x)G(x) = N(x) for any x∈Mx \in M, where N(x)N(x) is the unit normal vector of MM at xx. Let hh and gg denote the induced Riemannian metrics on MM and S2S^2 from R3\mathbb {R}^{3} respectively. Prove that if the mean curvature of MM is zero everywhere, then the Gauss map GG is a conformal map from (M,h)(M,h) to (S2,g)(S^2,g). (Recall: If (Σ1,g1)(\Sigma_1,g_1), (Σ2,g2)(\Sigma_2,g_2) are two Riemannian manifolds, a map ϕ:(Σ1,g1)→(Σ2,g2)\phi : (\Sigma_1,g_1) \to (\Sigma_2,g_2) is called conformal if g1=λϕ∗g2g_1 = \lambda \phi^*g_2 for some scalar function λ\lambda on Σ1\Sigma_1.)

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Problem 3.2.35

Let f:[a,b]→R+f : [a,b] \to \mathbb {R}^{}_+ be smooth, and let X⊂R3X \subset \mathbb {R}^{3} be the surface of revolution formed by revolving z=f(x)z=f(x) about xx-axis.

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(a)

For which function ff is the Gaussian curvature of XX

  • always positive?

  • always negative?

  • identically zero?

(b)

Characterize by a differential equation those functions ff such that XX is a minimal surface.

Problem 3.2.36

Let γ\gamma be a geodesic curve on a regular surface of revolution S⊂R3S \subset \mathbb {R}^{3}. Let θ(p)\theta (p) denote the angle the curve forms with the parallel at a point p∈γp \in \gamma and r(p)r(p) be the distance to the axis of revolution. Prove Clairaut's relation: rcos⁡θ=constr\cos \theta = \text{const}.

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Problem 3.2.37

Let F(x,y,z)F(x,y,z) be a smooth homogenous function of degree kk, i.e., F(λx,λy,λz)=λkF(x,y,z)F(\lambda x, \lambda y, \lambda z) = \lambda^k F(x,y,z). Prove that away from the origin, the induced metric on the conical surface Σ={(x,y,z)∣F(x,y,z)=0}\Sigma = \{ (x,y,z) \mid F(x,y,z) = 0\} has Gaussian curvature equal to 00.

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Problem 3.2.38

Let X⊂R3X \subset \mathbb {R}^{3} be the cone x2=y2+z2x^2=y^2+z^2, and let YY be the torus (x2+y2−2)2+z2=1(\sqrt{x^2+y^2}-2)^2+z^2=1, that is, the torus obtained by rotating the circle (x−2)2+z2−1=y=0(x-2)^2+z^2-1=y=0 around the zz-axis.

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(a)

Show that for any point p∈Xp \in X other than the vertex (0,0,0)(0,0,0), there is a neighborhood of pp in XX isometric to an open subset of the Euclidean plane R2\mathbb {R}^{2}.

(b)

Show that no open subset of YY is isometric to any open subset of the Euclidean plane.

Problem 3.2.39

Let Σ⊂R3\Sigma \subset \mathbb {R}^{3} be a smooth 2-dimensional submanifold, and n:Σ→R3n : \Sigma \to \mathbb {R}^{3} a smooth map such that n(p)n(p) is a unit length normal to Σ\Sigma at pp. Identify the tangent bundle TΣT\Sigma as the subspace of pairs (p,v)∈Σ×R3(p,v) \in \Sigma \times \mathbb {R}^{3} such that ⟨v,n(p)⟩=0\left\langle v, n(p) \right\rangle = 0. Suppose now the t→p(t)t \to p(t) is a smoothly parametrized curve in R3\mathbb {R}^{3} that lies on Σ\Sigma. Prove that this curve is a geodesic if and only if

p′′(t)⋅(n(p(t))×p′(t))=0, ∀t. p''(t) \cdot \bigl(n(p(t)) \times p'(t)\bigr) = 0, \, \forall t.

Here, p′p' is the derivative of the map t→p(t)t \to p(t) and p′′p'' is the second derivative.

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Problem 3.3.1

Let MnM^n be a Riemannian manifold and π\pi a 2-plane in T∗MT_*M.

?
(a)

Let {X,Y}\{ X,Y\} be an orthonormal basis of π\pi. Use this basis to define the sectional curvature K(π)K(\pi ) and show that it depends only on π\pi and not the particular basis chosen.

(b)

Define the Riemann curvature tensor in terms of covariant differentiation. Explain why it is a tensor.

(c)

Recall that if Mn⊂Rn+1M^n \subset \mathbb {R}^{n+1} is a hypersurface, then

R(X,Y)Z=⟨LY,Z⟩LX−⟨LX,Z⟩LY, R(X,Y)Z = \left\langle LY, Z \right\rangle LX - \left\langle LX, Z \right\rangle LY,

where LL is the Weingarten map. Using this or any other valid method, compute all sectional curvatures of the sphere {x∈R4:∣x∣=3}\{ x \in \mathbb {R}^{4} : \left|x\right|=3\}.

Problem 3.3.2

Let C={x∈R3:0≤xi≤1}C = \{ x \in \mathbb {R}^{3} : 0 \leq x_i \leq 1\} be the unit cube in R3\mathbb {R}^{3}. Suppose F:R3→R4F : \mathbb {R}^{3} \to \mathbb {R}^{4} is a 1−11-1 C∞C^\infty immersion in some neighborhood of CC. The image F(C)F(C) is then a compact Riemannian submanifold of R4\mathbb {R}^{4} with boundary and therefore has a volume. Justify the following formula:

vol⁡(F(C))=∫01∫01∫01∥F∗(∂∂x1)∧F∗(∂∂x2)∧F∗(∂∂x3)∥ dx1 dx2 dx3. \operatorname {vol}(F(C)) = \int _0^1\int _0^1\int _0^1 \left\| F_*\left(\frac{\partial }{\partial x_1}\right) \wedge F_*\left(\frac{\partial }{\partial x_2}\right) \wedge F_*\left(\frac{\partial }{\partial x_3}\right)\right\| \, dx_1 \, dx_2 \, dx_3.

Also, evaluate the integrand if

F(x)=((1+x1)2,(1+x2)2,(1+x3)2,(2+x3)3). F(x) = ((1+x_1)^2, (1+x_2)^2, (1+x_3)^2, (2+x_3)^3).
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Problem 3.3.3

Show that there is no submersion from S3S^3 into R2\mathbb {R}^{2}.

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Problem 3.3.4

Let MnM^n and NkN^k be Riemannian manifolds. Then M×NM \times N is naturally a Riemannian manifold with the product metric. If x1,…,xnx_1,\ldots ,x_n are local coordinates on MM and y1,…,yky_1,\ldots ,y_k are local coordinates on NN, the product metric in local coordinates (x1,…,xn,y1,…,yk)(x_1,\ldots ,x_n,y_1,\ldots ,y_k) looks like

g=(gij(x)00gpq(y)). g = \left(\begin{array}{c|c} g_{ij}(x) & 0 \\ \hline 0 & g_{pq}(y) \end{array}\right).
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(a)

Let XX be a vector field on M×NM \times N "along" MM (i.e., in local coordinates no ypy_p and ∂∂yq\dfrac {\partial }{\partial y_q} are present) and YY be a vector field along NN. Show that DXY≡0D_X Y \equiv 0.

(b)

Show that at z∈M×Nz \in M \times N, some sectional curvatures always vanish. (For example, product manifolds in the product metric never have strictly positive curvature.)

Problem 3.3.5

Let F:M→NF : M \to N be smooth, XX and YY be smooth vector fields on MM and NN, respectively, and assume F∗X=YF_*X = Y; that is, that

F∗p(X(p))=Y(F(p))for p∈M. F_{*p}(X(p)) = Y(F(p)) \qquad \text{for } p \in M.
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(a)

Let ω\omega be a smooth 1-form on NN. Define the Lie derivative LYωL_Y\omega of ω\omega with respect to YY. (If you use local coordinates, you must verify independence of choice of coordinates.)

(b)

Prove that

F∗(LYω)=LX(F∗ω). F^*(L_Y\omega ) = L_X(F^*\omega ).
(c)

Let ZZ be a smooth vector field on MM such that F∗Z=WF_*Z = W, where WW is a smooth vector field on NN. Show that LYW=F∗(LXZ)L_YW = F_*(L_XZ).

Problem 3.3.6

Let r,θ,zr,\theta ,z be the usual cylindrical coordinates in R3\mathbb {R}^{3}. Let

ω=[2rzsin⁡θ+3z2rcos⁡θ+5r2sin⁡2θ] dθ+[−2rcos⁡θ+6zrsin⁡θ] dz+[4zr2sin⁡θ] dr. \omega = [2rz\sin \theta + 3z^2r\cos \theta + 5r^2\sin ^2\theta ] \, d\theta + [-2r\cos \theta + 6zr\sin \theta ] \, dz + [4zr^2\sin \theta ] \, dr.

Let the curve γ\gamma be given in rectangular coordinates by

γ(t)=(x(t),y(t),z(t))=(cos⁡t,sin⁡t,4sin⁡5t+sin⁡2tcos⁡8t),0≤t≤2π. \gamma (t) = (x(t),y(t),z(t)) = (\cos t, \sin t, 4\sin ^5 t + \sin ^2 t\cos ^8 t), \qquad 0 \leq t \leq 2\pi .

Evaluate ∫γω\int_\gamma \omega.

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Problem 3.3.7

Let MM be a C∞C^\infty Riemannian manifold. Assume the theorem that there is a unique C∞C^\infty mapping ∇:X(M)×X(M)→X(M)\nabla : \mathcal{X}(M) \times \mathcal{X}(M) \to \mathcal{X}(M) denoted by ∇:(X,Y)→∇XY\nabla : (X,Y) \to \nabla_X Y which has the following linearity properties: For all f,g∈C∞(M)f,g \in C^\infty (M) and X,X′,Y,Y′∈X(M)X,X',Y,Y' \in \mathcal{X}(M), we have

_fX+gX’ Y = f(_X Y) + g(_X’ Y), _X(fY+gY') = f_X Y + g_X Y' + (Xf)Y + (Xg)Y', = _X Y - _Y X, X Y, Y' = _X Y, Y' + Y, _X Y' .

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(a)

Suppose α:[a,b]→M\alpha : [a,b] \to M is a smooth curve. Define what it means for a vector field YY on α\alpha to be parallel along α\alpha. Derive the differential equations that must be satisfied if YY is parallel along α\alpha.

(b)

Let X,Y∈X(M)X,Y \in \mathcal{X}(M). Let p∈Mp \in M and let α:[0,b]→M\alpha : [0,b] \to M be an integral curve of XX such that α(0)=p\alpha (0)=p, dα/dt=X(α(t))d\alpha /dt = X(\alpha (t)). Show that

(∇XY)(p)=ddt[Pα;0,t−1Y(α(t))]∣t=0, (\nabla _X Y)(p) = \frac{d}{dt}\bigl[P_{\alpha ;0,t}^{-1} Y(\alpha (t))\bigr]\Big|_{t=0},

where Pα;0,t:Tα(0)M→Tα(t)MP_{\alpha ;0,t} : T_{\alpha (0)}M \to T_{\alpha (t)}M is the parallel transport along α\alpha.

Problem 3.3.8

Let MM be a Riemannian manifold with the property that given any two points p,q∈Mp,q \in M the parallel transport of a vector from TpMT_pM to TqMT_qM is independent of the curve joining pp and qq. Prove that the curvature of MM is identically zero, i.e., R(X,Y)Z=0R(X,Y)Z=0 for all X,Y,Z∈X(M)X,Y,Z \in \mathcal{X}(M).

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Problem 3.3.9

Let MM be an nn-dimensional Riemannian manifold. Suppose there are nn orthonormal vector fields X1,…,XnX_1,\ldots ,X_n that commute with each other (i.e., [Xi,Xj]=0[X_i,X_j]=0; i,j=1,…,ni,j=1,\ldots ,n), show that the sectional curvature of MM is identically zero.

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Problem 3.3.10

Let XX be a smooth vector field on a Riemannian manifold MM. The divergence of XX, denoted by div⁡(X)\operatorname {div}(X), is defined by the function trace⁡(∇X)\operatorname {trace}(\nabla X).

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(a)

If MM is closed (i.e., compact without boundary), show that

∫Mdiv⁡(X) dv=0. \int _M \operatorname {div}(X) \, dv = 0.
(b)

If MM is compact with boundary ∂M\partial M, show that

∫Mdiv⁡(X) dv=∫∂M⟨X,N⟩ ds, \int _M \operatorname {div}(X) \, dv = \int _{\partial M} \left\langle X, N \right\rangle \, ds,

where NN is the outer normal vector field of ∂M\partial M.

Problem 3.3.11

Let ω1,…,ωk\omega^1,\ldots ,\omega^k be one-forms. Show that {ωi}i=1k\{ \omega^i\}_{i=1}^k are linearly independent if and only if ω1∧ω2∧⋯∧ωk≠0\omega^1 \wedge \omega^2 \wedge \cdots \wedge \omega^k \neq 0.

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Problem 3.3.12

Let MM be a Riemannian manifold. Let p∈Mp \in M.

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(a)

Show that there exists δ>0\delta > 0 such that

exp⁡p:Bδ(0)⊂TpM→M \exp _p : B_\delta (0) \subset T_pM \to M

is a diffeomorphism onto its image.

(b)

Show that there exists ε>0\varepsilon > 0 such that exp⁡p(Bε(0))\exp_p(B_\varepsilon (0)) is a convex set.

Problem 3.3.13

Let

A={(abcd):a,b,c,d∈R, ad−bc=1}. A = \left\{ \begin{pmatrix} a & b \\ c & d \end{pmatrix} : a,b,c,d \in \mathbb {R}, \, ad-bc=1\right\} .

Show that

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(a)

AA is a differentiable manifold.

(b)

AA is a Lie group with the standard matrix multiplication as a product.

Problem 3.3.14
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(a)

Let ff be a smooth function on a Riemannian manifold MM. Let grad⁡f\operatorname {grad} f be the vector field defined by the equation

⟨grad⁡f,v⟩p=dpf v,v∈TpM. \left\langle \operatorname {grad} f, v \right\rangle _p = d_pf \, v, \qquad v \in T_pM.

Let (x1,…,xn)(x^1,\ldots ,x^n) be local coordinates around pp. Find the expression for grad⁡f\operatorname {grad} f in terms of x1,…,xnx^1,\ldots ,x^n.

(b)

For a vector field XX define the divergence of XX, div⁡(X)\operatorname {div}(X) as the trace of the operator Y→DYXY \to D_Y X where DD is the Levi-Civita connection. Find the expression for the divergence of XX in a local coordinate system (x1,…,xn)(x^1,\ldots ,x^n).

(c)

Use (a) and (b) to find the expression for the Laplacian Δ\Delta in local coordinates, where Δ\Delta acting on a smooth function ff is defined by Δf=div⁡(∇f)\Delta f = \operatorname {div}(\nabla f).

Problem 3.3.15

Let MM be a compact connected Riemannian manifold without boundary. Let ff be a smooth function satisfying Δf=0\Delta f = 0. Show that f=constf = \text{const}.

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Problem 3.3.16

Suppose F:M→NF : M \to N is a smooth map between differentiable manifolds, and is homotopically trivial. Show that in this case, F∗ωF^*\omega will be exact whenever ω\omega is a closed 1-form on NN. [Note: FF is homotopically trivial if it extends to a smooth mapping Fˉ:M×[0,1]→N\bar F : M \times [0,1] \to N such that Fˉ(x,0)=F(x)\bar F(x,0) = F(x), for all x∈Mx \in M, while Fˉ(x,1)≡q∈N\bar F(x,1) \equiv q \in N (qq constant) for all xx.]

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Problem 3.3.17

Regard R9\mathbb {R}^{9} as the space of all 3×33\times 3 matrices with real entries. Does the subset

Σ={A∈R9:det⁡(A)=0} \Sigma = \{ A \in \mathbb {R}^{9} : \det (A) = 0\}

form a smooth submanifold of R9\mathbb {R}^{9}?

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Problem 3.3.18

Let

ω=x1 dx2∧dx3∧dx4+x2 dx1∧dx3∧dx4+x3 dx1∧dx2∧dx4. \omega = x_1 \, dx_2 \wedge dx_3 \wedge dx_4 + x_2 \, dx_1 \wedge dx_3 \wedge dx_4 + x_3 \, dx_1 \wedge dx_2 \wedge dx_4.

Compute ∫S3ω\int_{S^3} \omega, where S3={x∈R4:∣x∣=1}S^3 = \{ x \in \mathbb {R}^{4} : \left|x\right|=1\}, oriented as the boundary of the unit ball (assume standard orientation on R4\mathbb {R}^{4}).

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Problem 3.3.19

Prove that

{(x1,x2,x3,x4):rank⁡(x1x2x3x4)=1} \left\{ (x_1,x_2,x_3,x_4) : \operatorname {rank}\begin{pmatrix} x_1 & x_2 \\ x_3 & x_4 \end{pmatrix} = 1\right\}

is a three-dimensional submanifold of R4\mathbb {R}^{4}.

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Problem 3.3.20

Let vector fields X1,X2X_1, X_2 on R4\mathbb {R}^{4} be defined by

X1=∂∂x2+x1∂∂x3,X2=∂∂x1+x2∂∂x4. X_1 = \frac{\partial }{\partial x_2} + x_1\frac{\partial }{\partial x_3}, \qquad X_2 = \frac{\partial }{\partial x_1} + x_2\frac{\partial }{\partial x_4}.
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(a)

Is there a 2-dimensional submanifold M2M^2 of R4\mathbb {R}^{4} such that for each p∈M2p \in M^2, X1(p),X2(p)∈TpM2X_1(p), X_2(p) \in T_pM^2?

(b)

Is there a non-constant function ff in the neighborhood of 0∈R40 \in \mathbb {R}^{4} such that X1f≡0X_1 f \equiv 0 and X2f≡0X_2 f \equiv 0?

Problem 3.3.21

Let M={(x,y):x,y∈R3,∥x∥=1,∥y∥=1,⟨x,y⟩=0}M = \{ (x,y) : x,y \in \mathbb {R}^{3}, \left\| x\right\| =1, \left\| y\right\| =1, \left\langle x, y \right\rangle =0\}.

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(a)

Show that MM is a smooth compact embedded submanifold of R6\mathbb {R}^{6} and explain how MM can be identified with the unit tangent bundle of S2S^2.

(b)

Show that MM is orientable.

Problem 3.3.22

Let F:M→NF : M \to N be a local isometry between connected Riemannian manifolds MM and NN. Show that if MM is complete, so is NN and FF is a covering map.

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Problem 3.3.23

Let F:M→MF : M \to M be an isometry of a Riemannian manifold MM.

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(a)

Show that each component of X={x∈M:F(x)=x}X = \{ x \in M : F(x)=x\} is an embedded totally geodesic submanifold of MM.

(b)

Give an example in which the components of XX have different dimensions.

Problem 3.3.24

Compute the de Rham cohomology groups of the circle S1S^1. Do so directly; i.e., without citing the de Rham Theorem.

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Problem 3.3.25

Let XX denote a submanifold of Euclidean space En\mathbb {E}^n, and set

UεX:={x+v:x∈X,v∈NxX,∣v∣<ε},B(X,ε):={y∈En:∣y−x∣<ε for some x∈X}. \begin{align} U_\varepsilon X & := \{ x+v : x \in X, v \in N_xX, \left|v\right|<\varepsilon \} , \\ B(X,\varepsilon ) & := \{ y \in \mathbb {E}^n : \left|y-x\right|<\varepsilon \text{ for some } x \in X\} . \end{align}

Show that UεX⊂B(X,ε)U_\varepsilon X \subset B(X,\varepsilon ) for all ε\varepsilon. Show that the two are not generally equal. (Consider examples of 1-dimensional submanifold in E2\mathbb {E}^2.) Can you give conditions which imply equality?

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Problem 3.3.26

Consider a Riemannian manifold (M,g)(M,g). Call a vector field ZZ on MM a Killing vector field if ZZ generates a 1-parameter group of isometries of MM.

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(a)

Show that when ZZ is Killing, we have LZg=0L_Zg=0, i.e.,

Z(g(X,Y))=g(LZX,Y)+g(X,LZY)(**) Z(g(X,Y)) = g(L_ZX,Y) + g(X,L_ZY) \tag {**}

for all vector fields XX and YY on MM. Here LZgL_Zg denotes the Lie derivative along ZZ.

(b)

Show that the expression (**) above is equivalent to

g(∇XZ,Y)=−g(∇YZ,X), g(\nabla _XZ,Y) = -g(\nabla _YZ,X),

where ∇\nabla denotes the Levi-Civita connection for (M,g)(M,g).

Problem 3.3.27

Let M2M^2 be a connected Riemannian manifold and X,YX,Y complete vector fields on MM. Assume that the flows XtX_t and YtY_t are isometries of MM for all tt.

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(a)

Show that the integral curves of XX are curves of constant geodesic curvature.

(b)

Assume that XX and YY are linearly independent at all x∈M2x \in M^2 and that their flows commute Xt∘Ys=Ys∘XtX_t \circ Y_s = Y_s \circ X_t. Conclude that ⟨X,X⟩\left\langle X, X \right\rangle, ⟨X,Y⟩\left\langle X, Y \right\rangle and ⟨Y,Y⟩\left\langle Y, Y \right\rangle are constant on MM.

Problem 3.3.28

Let MM be a compact Riemannian manifold without boundary. For any f∈C∞(M)f \in C^\infty (M), define ∇f∈X(M)\nabla f \in \mathcal{X}(M) and Δf∈C∞(M)\Delta f \in C^\infty (M) as follows:

At any p∈Mp \in M, choose an orthonormal frame field {e1,…,en}\{ e_1,\ldots ,e_n\} around pp and then define

(∇f)(p)=∑i(eif)(ei) (\nabla f)(p) = \sum _i (e_if)(e_i)

and

(Δf)(p)=−∑i[ei(eif)−(∇eiei)f]. (\Delta f)(p) = -\sum _i [e_i(e_if) - (\nabla _{e_i}e_i)f].

Verify first that ∇f\nabla f and Δf\Delta f are well defined (i.e., they do not depend on the choice of orthonormal frame) and then show that

∫fΔf=∫∥∇f∥2. \int f\Delta f = \int \left\| \nabla f\right\| ^2.
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Problem 3.3.29

Let p(x1,x2,x3,x4)=(x12+x22)(x32+x42)p(x_1,x_2,x_3,x_4) = (x_1^2+x_2^2)(x_3^2+x_4^2) and q(x1,x2,x3,x4)=x12+x22+x32+x42q(x_1,x_2,x_3,x_4) = x_1^2+x_2^2+x_3^2+x_4^2. Define

Sa,b={x∈R4∣p(x)=a and q(x)=b}. S_{a,b} = \{ x \in \mathbb {R}^{4} \mid p(x)=a \text{ and } q(x)=b\} .

For what a,b≥0a,b \geq 0, is Sa,bS_{a,b} a manifold? Explain.

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Problem 3.3.30

Let F:M→NF : M \to N be a C∞C^\infty map between two C∞C^\infty manifolds. Assume that FF is onto. Let XX be a smooth vector field on MM.

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(a)

Show by an example that dF(X)dF(X) may not be a vector field on NN.

(b)

Suppose Y=dF(X)Y = dF(X) is a smooth vector field on NN. Show that FF takes integral curves of XX into integral curves of YY.

(c)

Suppose X1,Y1X_1,Y_1, and X2,Y2X_2,Y_2 are related as XX and YY in (b) above. Show that dF([X1,X2])=[Y1,Y2]dF([X_1,X_2]) = [Y_1,Y_2].

Problem 3.3.31

Let MnM^n be a Riemannian manifold. Show that whenever f:M→Rf : M \to \mathbb {R} is a smooth function, there is a unique vector field ∇f\nabla f (called the gradient of ff on MM) such that

⟨∇f(p),γ˙(t)⟩=ddtf(γ(t)) \left\langle \nabla f(p), \dot\gamma (t) \right\rangle = \frac{d}{dt} f(\gamma (t))

whenever γ\gamma is a smooth curve in MM with γ(t)=p\gamma (t) = p.

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Problem 3.3.32

The space Rn×n\mathbb {R}^{n\times n} of n×nn\times n real matrices forms an n2n^2-dimensional Euclidean space, in which the dot product between A=[aij]A=[a_{ij}] and B=[bij]B=[b_{ij}] is given by

⟨A,B⟩:=∑i=1n∑j=1naijbij. \left\langle A, B \right\rangle := \sum _{i=1}^n \sum _{j=1}^n a_{ij}b_{ij}.

Let Sn−1S^{n-1} be the unit sphere in Rn\mathbb {R}^{n}, and define σ:Sn−1→Rn×n\sigma : S^{n-1} \to \mathbb {R}^{n\times n} as the map sending x=(x1,…,xn)\mathbf{x} = (x_1,\ldots ,x_n) in Sn−1S^{n-1} to the symmetric matrix σ(x)=12[xixj]\sigma (\mathbf{x}) = \frac{1}{\sqrt2}[x_ix_j].

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(a)

Show that σ\sigma maps Sn−1S^{n-1} into the sphere of radius 12\frac{1}{\sqrt2} centered at the origin in Rn×n\mathbb {R}^{n\times n}.

(b)

Prove that σ\sigma is a local isometry (i.e., the pull-back via σ\sigma of the dot-product metric defined above on Rn×n\mathbb {R}^{n\times n} is the standard one on Sn−1S^{n-1}).

Problem 3.3.33

Let MM be the Riemannian manifold obtained by equipping Rn\mathbb {R}^{n} with a metric conformal to its usual one; i.e., a metric of the form [gij]=e2f[δij][g_{ij}] = e^{2f}[\delta_{ij}], where f:Rn→Rf : \mathbb {R}^{n} \to \mathbb {R} is a smooth function, and δij\delta_{ij} is the Kronecker delta. Let ei=∂∂xie_i = \dfrac {\partial }{\partial x_i} denote the standard coordinate basis vector fields.

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(a)

Show that for arbitrary indices i,j,k∈{1,2,…,n}i,j,k \in \{ 1,2,\ldots ,n\}

⟨∇eiej,ek⟩=e2f(∂f∂xiδjk−∂f∂xkδij+∂f∂xjδki). \left\langle \nabla _{e_i}e_j, e_k \right\rangle = e^{2f}\left(\frac{\partial f}{\partial x_i}\delta _{jk} - \frac{\partial f}{\partial x_k}\delta _{ij} + \frac{\partial f}{\partial x_j}\delta _{ki}\right).
(b)

Show that when n=2n=2, the sectional curvature of MM along an e1,e2e_1,e_2 plane at pp is given by

−e−2f(p)(∂2f∂x12+∂2f∂x22)(p). -e^{-2f(p)}\left(\frac{\partial ^2 f}{\partial x_1^2} + \frac{\partial ^2 f}{\partial x_2^2}\right)(p).
Problem 3.3.34

Let X,YX,Y be complete vector fields on a manifold MM and let Xt,YtX_t,Y_t be the flows induced by them.

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(a)

Show that Xs∘Yt=Yt∘XsX_s \circ Y_t = Y_t \circ X_s for all s,t∈Rs,t \in \mathbb {R} implies [X,Y]=0[X,Y]=0.

(b)

Prove the converse to (a).

Problem 3.3.35

If ϕ:G1→G2\phi : G_1 \to G_2 is a Lie group homomorphism, show that for all v∈LG1v \in LG_1, we have

ϕ(exp⁡(v))=exp⁡(ϕ∗v). \phi (\exp (v)) = \exp (\phi _*v).
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Problem 3.3.36

Consider the linearly independent vector fields r\mathbf{r} and v\mathbf{v} on U:=R4∖0U := \mathbb {R}^{4}\setminus 0 whose values at x=(x1,x2,x3,x4)∈R4\mathbf{x} = (x_1,x_2,x_3,x_4) \in \mathbb {R}^{4} are given by

rx:=(x1,x2,x3,x4),vx:=(−x2,x1,−x4,x3). \begin{align} \mathbf{r}_x & := (x_1,x_2,x_3,x_4), \\ \mathbf{v}_x & := (-x_2,x_1,-x_4,x_3). \end{align}
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(a)

Is the rank-2 distribution defined by these two vector fields in UU completely integrable?

(b)

Is the rank-2 distribution orthogonal to these two vector fields completely integrable?

Problem 3.3.37

Let GG be a Riemannian manifold with a global frame-field {ei}i=1n\{ e_i\}_{i=1}^n.

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(a)

Show that any connection on GG is completely determined by its effect on the frame field, i.e., by the vector fields ∇eiej\nabla_{e_i}e_j, i,j=1,…,ni,j=1,\ldots ,n.

(b)

Show that when GG is a Lie group with a bi-invariant metric ⟨⋅,⋅⟩\left\langle \cdot , \cdot \right\rangle, and the frame-field is left-invariant, we characterize the Levi-Civita connection on (G,⟨⋅,⋅⟩)(G, \left\langle \cdot , \cdot \right\rangle ) by setting,

∇eiej=12[ei,ej] \nabla _{e_i}e_j = \frac12 [e_i,e_j]

for all i,j=1,…,ni,j=1,\ldots ,n.

Problem 3.3.38

Let ϕ:Rn→Rn\phi : \mathbb {R}^{n} \to \mathbb {R}^{n} be any isometry, that is, a map such that the Euclidean distance between any two points x,y∈Rnx,y \in \mathbb {R}^{n} is equal to the distance between their images ϕ(x),ϕ(y)\phi (x), \phi (y). Show that ϕ\phi is affine linear, that is, there exists a vector b∈Rnb \in \mathbb {R}^{n} and an orthogonal matrix A∈O(n)A \in O(n) such that for all x∈Rnx \in \mathbb {R}^{n}, ϕ(x)=Ax+b\phi (x) = Ax+b.

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Problem 3.3.39

Show that the sphere S2nS^{2n} is not the underlying topological space of any Lie group.

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Problem 3.3.40

Let U⊂R2U \subset \mathbb {R}^{2} be an open set.

?
(a)

Define a Riemannian metric on UU.

(b)

In terms of your definition, define the distance between two points p,q∈Up,q \in U.

(c)

Let Δ={(x,y):x2+y2<1}\Delta = \{ (x,y) : x^2+y^2<1\} be the open unit disc in R2\mathbb {R}^{2}, and consider the metric on Δ\Delta given by

ds2=dx2+dy2(1−x2−y2)2. ds^2 = \frac{dx^2+dy^2}{(1-x^2-y^2)^2}.

Show that Δ\Delta is complete with respect to this metric.

Problem 3.3.41

Let H={(u,v)∈R2∣v>0}H = \{ (u,v) \in \mathbb {R}^{2} \mid v>0\} and B={(x,y)∈R2∣x2+y2<1}B = \{ (x,y) \in \mathbb {R}^{2} \mid x^2+y^2<1\}. For e2=(0,1)∈R2e_2=(0,1) \in \mathbb {R}^{2}, map HH to BB by the following diffeomorphism

v↦x=−e2+2(v+e2)∥v+e2∥2. \mathbf{v} \mapsto \mathbf{x} = -e_2 + \frac{2(\mathbf{v}+e_2)}{\left\| \mathbf{v}+e_2\right\| ^2}.
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(a)

Verify that the image of the above map is indeed BB.

(b)

Consider the following metric on BB:

g=dx2+dy2(1−∥x∥2)2. g = \frac{dx^2+dy^2}{(1-\left\| \mathbf{x}\right\| ^2)^2}.

Put a metric on HH such that the above map is an isometry.

(c)

Show that HH is complete.

Problem 3.3.42

Define a metric on the unit disc {(x,y)∈R2:x2+y2<1}\{ (x,y) \in \mathbb {R}^{2} : x^2+y^2<1\} by the line element

ds2=dρ2+ρ2dθ2(1−ρ2)p. ds^2 = \frac{d\rho ^2 + \rho ^2 d\theta ^2}{(1-\rho ^2)^p}.

Here (ρ,θ)(\rho ,\theta ) are polar coordinates and pp is any real number.

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(a)

For which pp is the circle ρ=1/2\rho =1/2 a geodesic?

(b)

Compute the Gaussian curvature of this metric.

Problem 3.3.43

Let (H2,g)(\mathbb {H}^2, g) be the two-dimensional hyperbolic space, where

H2={(x,y)∈R2:y>0} \mathbb {H}^2 = \{ (x,y) \in \mathbb {R}^{2} : y>0\}

is the upper half plane of R2=C\mathbb {R}^{2} = \mathbb {C} and the metric gg is given by

g=dx2+dy2y2. g = \frac{dx^2+dy^2}{y^2}.
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(a)

Suppose a,b,ca,b,c and dd are real numbers such that ad−bc=1ad-bc=1. Define

ϕ(z)=az+bcz+d \phi (z) = \frac{az+b}{cz+d}

for any z=x+−1yz = x+\sqrt{-1}y. Prove that ϕ\phi is an isometry for (H2,g)(\mathbb {H}^2,g).

(b)

Prove that (H2,g)(\mathbb {H}^2,g) has constant Gaussian curvature.

Problem 3.3.44

Suppose that ∇\nabla is a connection on a Riemannian manifold MM. Define the torsion tensor τ\tau via τ(X,Y)=∇XY−∇YX−[X,Y]\tau (X,Y) = \nabla_XY - \nabla_YX - [X,Y], where X,YX,Y are vector fields on MM. ∇\nabla is called symmetric if the torsion tensor vanishes. Show that ∇\nabla is symmetric if and only if the Christoffel symbols with respect to any coordinate frame are symmetric, i.e., Γijk=Γjik\Gamma_{ij}^k = \Gamma_{ji}^k. Remember that if {Ei}\{ E_i\} is a coordinate frame, and ∇\nabla is a connection, the Christoffel symbols are defined via

∇EiEj=∑kΓijkEk. \nabla _{E_i}E_j = \sum _k \Gamma _{ij}^k E_k.
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Problem 3.3.45
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(a)

Consider Rn\mathbb {R}^{n} with the standard Euclidean metric and let p∈Rnp \in \mathbb {R}^{n} be an arbitrary point. For any x∈Rnx \in \mathbb {R}^{n} let ρp(x)\rho_p(x) be the distance from pp to xx. Viewing ρp(x)\rho_p(x) as a smooth function of xx away from pp, verify that ∣grad⁡(ρp(x))∣2=1\left|\operatorname {grad}(\rho_p(x))\right|^2 = 1 and that the integral curves of grad⁡(ρp(x))\operatorname {grad}(\rho_p(x)) are straight lines. (Here grad⁡(ρp(x))\operatorname {grad}(\rho_p(x)) refers to the usual gradient vector field of the function ρp(x)\rho_p(x).)

(b)

More generally, given a smooth function ff on a Riemannian manifold (M,gij)(M,g_{ij}), define grad⁡(f)\operatorname {grad}(f) to be the vector field given locally by

∑i,j(gij∂f∂xj)∂∂xi \sum _{i,j} \left(g^{ij}\frac{\partial f}{\partial x^j}\right)\frac{\partial }{\partial x^i}

show that if ∣grad⁡(f)∣2=1\left|\operatorname {grad}(f)\right|^2=1, then the integral curves of the vector field grad⁡(f)\operatorname {grad}(f) are geodesics.